First-order phase transitions between 1 and 10^6 GeV can simultaneously source LISA-detectable gravitational waves and intergalactic magnetic fields matching MAGIC bounds when a fraction of sound-wave energy converts to MHD turbulence.
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LISA and $\gamma$-ray telescopes as multi-messenger probes of a first-order cosmological phase transition
First-order phase transitions between 1 and 10^6 GeV can simultaneously source LISA-detectable gravitational waves and intergalactic magnetic fields matching MAGIC bounds when a fraction of sound-wave energy converts to MHD turbulence.